Origin of Life Flashcards

(60 cards)

1
Q

List the seven shared biological characteristics of all living organisms.

A

Cellular organisation; hierarchical organisation; energy use; response to stimuli; growth; reproduction; adaptation/homeostasis

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2
Q

Give the seven shared chemical characteristics of life.

A

Carbon-based; energy use; redox gradients; proteins–lipids–carbohydrates; nucleic-acid heredity; ATP as energy currency; core metabolic pathways conserved

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3
Q

How old is the Universe and the Earth?

A

Universe ≈ 13.7 billion years; Earth ≈ 4.55 billion years

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4
Q

What event likely formed the Moon and when?

A

Giant impact with protoplanet Thea ≈ 75 million years after Earth’s formation

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5
Q

What is the Late Heavy Bombardment and its biological significance?

A

4.1–3.8 bya barrage of meteorites/comets that sterilised surface yet delivered water & organics

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6
Q

Name three harsh features of the Hadean Earth.

A

5-h day length; acidic oceans with ~30 m tides & frequent boiling; anaerobic toxic atmosphere full of dust/ash

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7
Q

Earliest robust evidence for life appears at what age?

A

Carbon isotope signatures ≈ 3.8 bya; stromatolite-like fossils ≈ 3.5 bya

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8
Q

List six historical hypotheses for life’s origin

A

Panspermia, mineral clays, volcano/ice variants, primordial soup, acidic deep-sea vents, alkaline hydrothermal vents

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9
Q

What did meteorite ALH 84001 once appear to show?

A

Possible microfossils from Mars (later judged abiotic)

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10
Q

2023 Ryugu asteroid finding relevant to panspermia?

A

Detection of uracil and niacin—prebiotic organics—implying delivery of bases to Earth

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11
Q

Summarise the Miller-Urey apparatus and outcome.

A

Simulated reducing atmosphere (H₂, CH₄, NH₃, H₂O) + electric sparks → amino acids via formaldehyde pathway

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12
Q

Give two major criticisms of the original primordial-soup model.

A

(1) Early atmosphere likely CO₂/N₂-rich, not strongly reducing. (2) Dilution & energy issues—compounds too dispersed, lightning both creates & destroys organics

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13
Q

Define the “concentration problem” in origin-of-life research.

A

Reactants must accumulate locally at high enough concentrations to react and replicate; open ocean is too dilute

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14
Q

Contrast black-smoker acidic vents with alkaline vents.

A

Acidic smokers are high-temp, O₂-poor, near redox equilibrium; alkaline vents supply H₂, natural pH gradient, Fe-S catalysts, and microporous chambers to concentrate chemistry

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15
Q

What geological process generates alkaline vents?

A

Serpentinisation: seawater infiltrates upper mantle, forming serpentine rock and releasing alkaline, H₂-rich fluids

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16
Q

Why are proton gradients central to the alkaline-vent hypothesis?

A

Vent pH ~10–11 vs acidic early ocean pH ~5–6 → natural ΔpH could drive ATP-like chemistry before membranes evolved

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17
Q

Name four features of alkaline vents that solve the concentration problem.

A

Microporous Fe-S-lined chambers; continuous flow reactors; H₂/CO₂ redox power; mineral walls as catalysts & semi-permeable barriers

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18
Q

What modern field site exemplifies alkaline-vent structures?

A

The “Lost City” hydrothermal field on Atlantis Massif (discovered 2000)

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19
Q

Why examine LUCA when probing life’s origins?

A

Shared biochemical traits of all extant life set a minimum feature-set and hint at the environment/chemistry where life began

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20
Q

Single-sentence summary: why do alkaline vents currently lead origin-of-life models?

A

“They uniquely combine compartmentalisation, sustained H₂/CO₂ redox energy, Fe-S catalysis, and natural proton gradients—

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21
Q

What is LUCA and why do we study it?

A

LUCA = Last Universal Common Ancestor; the shared biochemical toolkit of all life lets us infer the environment and chemistry present when cellular life first emerged.

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22
Q

Why is LUCA unlikely to have been free-living?

A

It was probably confined within mineral ‘cells’ of alkaline hydrothermal vents, which supplied concentration, catalysts, and a proton gradient instead of a self-made membrane.

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23
Q

Which biomolecule could both store information and catalyse reactions making it the best candidate before DNA and protein?

A

RNA

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24
Q

Give two arguments for RNA preceding protein.

A

(1) Ribozymes show RNA can catalyse reactions; (2) an RNA strand can carry sequence information needed to specify peptides.

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25
Give two arguments for RNA preceding DNA.
(1) No universally conserved DNA-replication enzymes—bacteria and archaea use different machineries, implying DNA arose after their split; (2) DNA shows no catalytic activity, whereas RNA does.
26
What discovery did Walter Gilbert (1986) highlight to support an RNA world?
Several RNAs (self-splicing introns, transposon RNAs) already act as enzymes, suggesting ancient catalytic roles.
27
How can a two-nucleotide “code” catalyse amino-acid synthesis?
First base specifies precursor (e.g., C = α-ketoglutarate), second base specifies product property (e.g., U = hydrophobic AA), allowing dinucleotides to act like mini-tRNAs.
28
Where do vents supply the high concentrations needed for spontaneous RNA polymerisation?
Microporous chambers concentrate nucleotides; convection/thermal cycling acts like PCR, promoting chain extension.
29
What natural gradient in alkaline vents could power early metabolism?
A pH (proton) gradient: alkaline vent fluid (~pH 10) meets acidic Hadean ocean (~pH 5-6), generating ΔpH across chimney walls.
30
What alternative energy carrier may have preceded ATP in vent chemistry?
Acetyl phosphate or other acetyl thioesters storing energy from H₂ + CO₂ redox before ATP synthase evolved.
31
Why is ATP especially suited once proton gradients were harnessed?
ATP formation couples to proton flow (≈4 H⁺ per ATP), providing a reusable energy ‘currency’ for diverse reactions.
32
What key metabolic cycle can run in reverse under vent-like conditions to build carbon compounds?
The reverse (reductive) tricarboxylic-acid (TCA) cycle.
33
How does the Martin–Russell theory connect vents to early carbon fixation?
Fe-S and Ni catalysts in vent minerals enable H₂ + CO₂ → acetyl groups, feeding into reverse TCA chemistry.
34
What structural innovation allowed descendants of LUCA to leave the vent?
Development of a self-made membrane, initially peptide-lined bubbles that later evolved into lipid bilayers.
35
Why do bacterial and archaeal membranes differ fundamentally (ester- vs ether-linked lipids)?
Membrane evolution occurred independently after their divergence, supporting a post-LUCA origin of modern lipid types.
36
Which metabolism-based lineages represent early divergences after LUCA?
Acetogens (acetate producers) and methanogens (methane producers), both vent-dwelling anaerobes using membrane-bound chemiosmosis.
37
What evidence suggests DNA evolved from RNA not vice versa?
Enzymes for making deoxyribose and thymine can be derived from ribose and uracil, pointing to biochemical modification of RNA components.
38
Why is DNA favourable once it appears despite RNA’s versatility?
Greater chemical stability and double-strand templating allow longer genomes and more accurate replication.
39
Summarise the “bioreactor” concept of early life.
Early vent ‘cells’ acted as continuous-flow reactors where RNA, peptides, and small-molecule metabolism co-evolved before true free-living cells emerged.
40
Give the lecture’s sequence of key evolutionary transitions.
Vent mineral cell → catalytic/self-replicating RNA → RNA-directed peptide synthesis → DNA genomes → ATP chemiosmosis → lipid membranes → free-living bacteria & archaea.
41
What is the Great Oxygenation Event (GOE)?
A rapid rise in atmospheric O₂ between ≈2.45–2.2 billion years ago, linked to oxygenic photosynthesis and evidenced by sulfur-isotope shifts and global iron ‘rusting’.
42
List three independent lines of evidence for the GOE.
(1) Mass-independent sulfur-isotope fractionation ends; (2) banded-iron formations/‘Great Rusting’; (3) geochemical O₂ proxies in shales/carbonates show step-increase.
43
Which organisms are credited with triggering the GOE?
Oxygenic cyanobacteria performing water-splitting photosynthesis.
44
Why is there a ≈300 Myr time lag between first cyanobacterial fossils (≈2.7 Ga) and bulk O₂ rise (≈2.45 Ga)?
Early O₂ was buffered by reduced volcanic gases, dissolved iron, and sulfate; significant accumulation required sinks to saturate/decline.
45
State two additional geological factors (besides biology) that aided O₂ accumulation.
(1) Decrease in mantle melting reduced outgassing of O₂-reactive gases. (2) Tectonic compositional change lowered reductant supply to oceans/atmosphere.
46
Explain how rising O₂ could trigger a global ‘Snowball Earth’.
O₂ oxidised CH₄ (a strong greenhouse gas) to CO₂ (weaker), reducing greenhouse warming and causing planetary glaciations (Huronian & Makganyene).
47
Name two major biological consequences of the GOE.
(1) Extinction or retreat of anaerobes; (2) opening niches for aerobic respiration and later eukaryotic evolution.
48
Why does photosynthesis provide a competitive advantage to vent-emigrant microbes?
It supplies both reducing power and proton gradients using abundant sunlight, replacing vent chemiosmosis.
49
Define photosynthesis in metabolic terms.
Light-driven generation of ATP and NADPH to reduce and assimilate CO₂ into carbohydrates.
50
What three resources must primitive photosynthesis supply to fix CO₂?
Energy (light-harvest), reducing power (electron donor/NADPH), and an enzyme catalyst (e.g., RuBisCO) with a suitable carbon-acceptor substrate.
51
Describe the role of Photosystem I vs Photosystem II in bacteria.
PS I generates a powerful reductant for NAD(P)⁺; PS II creates a proton gradient and, in oxygenic lineages, extracts electrons from water.
52
What unique cofactor enables PS II to split water?
The oxygen-evolving complex (OEC), a Mn₄CaO₅ cluster tethered to a tyrosine that stores and releases four oxidising equivalents.
53
Why is manganese thought to pre-adapt photosynthetic water splitting?
Mn minerals in vents can cycle multiple valence states and absorb high-energy electrons; OEC’s (oxygen evolving complex) structure mimics vent manganese oxides.
54
Outline the hypothesised sequence of photosystem evolution in prokaryotes.
Independent single photosystems (PS I-like or PS II-like) → gene fusion/duplication → combined two-photosystem apparatus in cyanobacteria.
55
All modern photosystems share what two structural features?
(1) A reaction-centre core of homologous proteins; (2) bound (bacterio)chlorophyll pigments for light absorption.
56
Why do different bacteria use distinct pigments?
Diverse pigments tune light absorption to ecological niches yet retain a common tetrapyrrole backbone, indicating shared ancestry with haem.
57
Give one reason photosynthesis may have evolved on land/shallow water.
High UV/light exposures offer abundant energy, and surface Mn/Fe minerals could facilitate early photochemistry.
58
Explain why selective loss and fusion events complicate tracing photosystem ancestry.
Genes encoding reaction centres can be lost, duplicated, or rearranged, producing varied present-day combinations despite shared origins.
59
What is the functional payoff of combining PS I and PS II into a tandem ‘Z-scheme’?
Sequential light hits boost electron energy twice, enabling extraction from water and production of both ATP and strong reductant (NADPH).
60
Summarise the lecture’s key take-home message in one sentence.
Early photosystems evolved to create independent proton gradients; their water-splitting upgrade oxygenated the planet, driving catastrophic climate shifts and paving the way for complex life.